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Brian E. Brumfield † Susanna Widicus Weaver ‡ Claire Gmachl * Scott Howard* Benjamin McCall ‡ High-Resolution cw-CRDS of the ν 8 Band of Methylene Bromide †Department of Chemistry, University of Illinois at Urbana-Champaign, Urbana, IL 61801 ‡Departments of Chemistry and Astronomy, University of Illinois at Urbana-Champaign, Urbana, IL 61801 *Department of Electrical Engineering, Princeton University, Princeton Institute for the Science and Technology of Materials, Princeton, NJ, 08544
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Overview Introduction Motivation for spectroscopy of CH 2 Br 2 Experimental CH 2 Br 2 General details Spectra/simulations Conclusions
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Why CH 2 Br 2 ? Needed temperature probe of supersonic expansion for C 60 project Requirements Need an accessible vibrational band ~1185-1198 cm -1 (~8.5 μm) The band should cover a reasonably small window in frequency space ~5 cm -1 A relatively simple molecule that is liquid or gas phase at room temperature. Only ν 8 band of CH 2 Br 2 reasonably fit the requirements Band center ν 0 ~1195 ± (1-3) cm -1 Strong band No high-resolution spectrum available 1194 cm -1 (CD3)2HfD2(CD3)2HfD2 1194 cm -1 ZnZnDZnZnD 1194 cm -1 F2C=C=C=OF2C=C=C=O 1194 cm -1 F2C=C=CFCF:F2C=C=CFCF: 1195 cm -1 Boron dicarbideBoron dicarbide 1195 cm -1 CuCuD-CuCuD- 1195 cm -1 (N)2(cyc-C3N3)N3(N)2(cyc-C3N3)N3 1195 cm -1 p-C6H4ClNH2+p-C6H4ClNH2+ 1195 cm -1 NSONSO 1195 cm -1 DCFDCF 1195 cm -1 Ga2H6Ga2H6 1195 cm -1 MethylamineMethylamine 1195 cm -1 Methane, dibromo-Methane, dibromo- 1195 cm -1 (CH3)2Ge(CH3)2Ge 1195 cm -1 C2H5IOC2H5IO 1195 cm -1 CCl2+CCl2+ 1196 cm -1 ZnZnDZnZnD 1196 cm -1 Cl3TiOCD3Cl3TiOCD3 1196 cm -1 1,3-Butadiene-d61,3-Butadiene-d6 1196 cm -1 1,3-Butadiene1,3-Butadiene 1196 cm -1 1,2,4-Trioxolane1,2,4-Trioxolane 1196 cm -1 C6F6+C6F6+ 1196 cm -1 HCOOH+HCOOH+ 1196 cm -1 HCClBrHCClBr 1196 cm -1 CH3CCCl+ CH3CCCl+ Nist Chemistry WebBook. webbook.nist.gov/chemistry/
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Experimental Overview Cryostat with QCL Aspheric Lens Mode-matching optics High finesse cavity Focusing optics & detector AOM N 2 O Reference cell Reference Detector
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Experimental:Laser Limited commercial availability ~8 μm Quantum cascade laser Multi-quantum well design- Like a particle in a box Wavelength coverage not as strongly tied to band-gap of materials ~80 mW attainable cw output power Energy Valence Band Conduction Band h =ΔE gap Ordinary Diode Laser Energy Position Quantum Cascade Laser
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Laser Visual Bias Voltage Common Ground 5-7 Lasers Per Chip
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Laser Housing/Mounting Cold Plate (77 K) Copper Ribbon for Thermal Conductivity but Mechanical Isolation “Sample Mount” Armature for Mechanical Rigidity On Reverse: Heater & Temp. Sensor Laser Mount Janis VPF-100
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Laser Tuning Frequency tuning carried out by manipulating I and T of laser
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cw-CRDS cw-light coupled into cavity Resonance-light intensity in cavity builds up Threshold-source uncoupled via AOM deflection Exponential decay of light from cavity measured Rate of decay depends on: Mirror losses Absorbing species present Can back out absorption coefficient
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Supersonic Expansion Rotational/Vibrational cooling of sample carried out in a supersonic expansion. 0.7 mm pinhole expansion source Normal experimental pressures P o /P 1 ~ 1.7 x 10 4 Sample delivery by bubbling Ar carrier gas through liquid CH 2 Br 2 C 60 CH 2 Br 2 + Ar
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CH 2 Br 2 General Details % Abundance of 79 Br and 81 Br is 50/50 Three isotopomers present in sample spectral congestion Low symmetry weak dependence of intensity w.r.t. nuclear spin statistics of CH 2 79 Br 2 and CH 2 81 Br 2 CH 2 79 Br 2 CH 2 79 Br 81 BrCH 2 81 Br 2 % Sample25%50%25% Point Group Symmetry C 2v CsCs
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CH 2 Br 2 Ground Rotational Constants Microwave work exists for all three isotopomers Ray’s Asymmetry Parameter: Near prolate top Spectral simplification Rotational Constant CH 2 79 Br 2 * CH 2 79 Br 81 Br ** CH 2 81 Br 2 * A” (MHz)26031.31426007.57025984.704 B” (MHz)1238.53671223.29461208.0839 C” (MHz)1190.94201176.79571162.6650 κ -0.99617-0.99625-0.99634 *Davis W.R. and Gerry M.C.L. J. Mol. Spec. 109, 269-282 (1985) **Niide et al. J. Mol. Spec. 139, 11-29 (1990) a
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CH 2 Br 2 Rovibrational Details ν 8 -CH 2 wag rovibrational band characteristics: ║ vibrational band (Q-branch expected) 3 distinct band-centers for each isotopomer ~1197 cm -1 a-type transitions Selection Rules: ΔJ=0,±1 ; ΔK a =0 ; ΔK c =±1 a
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CH 2 Br 2 Spectra Calibrated 1195.81 cm -1 to 1196.96 cm -1 Laser Frequency Step: 50 MHz
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Spectra Compared To 15K Simulation A′=25890 MHz B′=1208 MHz C′=1178 MHz ν 0 =1196.98 cm -1 QQ1QQ1 QQ2QQ2 QQ3QQ3 QQ5QQ5 QQ4QQ4
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Spectra Compared To 35K Simulation A′=25890 MHz B′=1208 MHz C′=1178 MHz ν 0 =1196.98 cm -1 QQ2QQ2 QQ1QQ1 QQ3QQ3 QQ4QQ4 QQ5QQ5
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Conclusions High resolution spectroscopy of the methylene bromide v 8 band has been carried out Preliminary work has provided a tentative assignment for the Q-branch of the CH 2 79 Br 81 Br isotopomer Assessment of Q-branch features provides a rough diagnostic for the temperature of our supersonic expansion More scanning needs to be done: Beyond 1197 cm -1 encompass a sufficient portion of the R branch At 35 MHz step size
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Acknowledgements NASA Laboratory Astrophysics Rich Saykally (UC Berkeley) Dreyfus UIUC David Plusquellic-JB95 Fitting Package David Woon-Vibration/Rotation Animations Susanna Widicus Weaver Brett McGuire
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